Contraction of radiating shell in classical and Post-Newtonian approximation
A semi-numeric method was used to study the evolution of a general-relativistic radiating shell in its Post-Newtonian and Newtonian approximations. The solutions, where the main parameters are given reasonable values, show that a relativistic effect can be found in X-ray-burster-like objects.
Guardado en:
| Publicado: |
1999
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004640X_v268_n4_p469_Santoro http://hdl.handle.net/20.500.12110/paper_0004640X_v268_n4_p469_Santoro |
| Aporte de: |
| Sumario: | A semi-numeric method was used to study the evolution of a general-relativistic radiating shell in its Post-Newtonian and Newtonian approximations. The solutions, where the main parameters are given reasonable values, show that a relativistic effect can be found in X-ray-burster-like objects. |
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